DIXE proposes CSS-based survey strategies covering 72.5% of the sky with 26-68 ks exposures and shows via simulation that MCMC collimator demodulation yields 1° point-source localization and 3° extended-source resolution.
Title resolution pending
8 Pith papers cite this work, alongside 207 external citations. Polarity classification is still indexing.
8
Pith papers citing it
207
external citations · OpenAlex
verdicts
UNVERDICTED 8representative citing papers
U-Net inversion of red-clump extinction yields Galactic-plane dust density maps to 7 kpc with a 2.90 kpc exponential scale length and M74-like spiral morphology.
Analysis of 3161 molecular clouds reveals oblate shapes aligned with the galactic plane, a flatter velocity dispersion-size relation than Larson's law, strong mass-size correlation, and that 12CO traces diffuse turbulent gas while C18O traces gravity-dominated regions.
Three-dimensional three-temperature simulations of colliding supersonic plasma flows from irradiated CH mesh targets produce a persistent shocked turbulent mixing layer that evolves toward an isothermal state with anisotropic Reynolds stress and effective Reynolds number around 200.
Time-dependent cosmic ray electron spectra in a simulated galactic disk match steady-state solutions up to 500 GeV but become steeper and more disk-confined at higher energies due to recent injections.
Proposal for SKA-Low survey to perform 3D tomography of the Local Bubble's magnetized gas using polarized emission and rotation measure synthesis.
Simulations of an NGC 300-like galaxy find exponential distributions of feedback-driven bubble lifetimes and sizes that increase with galactocentric radius, plus matching Hα predictions.
FAST observations of three pulsars detect scintillation arcs whose curvatures scale as ν^{-2} with frequency, locating scattering screens at 30-420 pc.
citing papers explorer
-
DIffuse X-ray Explorer (DIXE): Sky Survey Strategy and Collimator Response Demodulation
DIXE proposes CSS-based survey strategies covering 72.5% of the sky with 26-68 ks exposures and shows via simulation that MCMC collimator demodulation yields 1° point-source localization and 3° extended-source resolution.
-
A Face-on View of Interstellar Dust in the Galactic Plane
U-Net inversion of red-clump extinction yields Galactic-plane dust density maps to 7 kpc with a 2.90 kpc exponential scale length and M74-like spiral morphology.
-
Statistical Properties of Molecular Clouds in the Milky Way: Insights from Three-Isotopologue CO Observations of the MWISP Project
Analysis of 3161 molecular clouds reveals oblate shapes aligned with the galactic plane, a flatter velocity dispersion-size relation than Larson's law, strong mass-size correlation, and that 12CO traces diffuse turbulent gas while C18O traces gravity-dominated regions.
-
Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas
Three-dimensional three-temperature simulations of colliding supersonic plasma flows from irradiated CH mesh targets produce a persistent shocked turbulent mixing layer that evolves toward an isothermal state with anisotropic Reynolds stress and effective Reynolds number around 200.
-
Steady-State or Not? The Evolution of Cosmic Ray Electron Spectra in Galaxies
Time-dependent cosmic ray electron spectra in a simulated galactic disk match steady-state solutions up to 500 GeV but become steeper and more disk-confined at higher energies due to recent injections.
-
A 3D tomography of the Local Bubble with SKA-Low
Proposal for SKA-Low survey to perform 3D tomography of the Local Bubble's magnetized gas using polarized emission and rotation measure synthesis.
-
Unmasking Stellar Feedback-Driven Bubbles: Identification and Properties Analysis
Simulations of an NGC 300-like galaxy find exponential distributions of feedback-driven bubble lifetimes and sizes that increase with galactocentric radius, plus matching Hα predictions.
-
Interstellar Scintillation of Three Nearby Pulsars with FAST
FAST observations of three pulsars detect scintillation arcs whose curvatures scale as ν^{-2} with frequency, locating scattering screens at 30-420 pc.